Rosa M. González Delgado

TL;DR: The detection, in Hα emission, of a radial corrugation in the velocity field of the spiral galaxy NGC 5427 shows kinematical behavior similar to the one expected in a galactic bore generated by the interaction of a spiral density wave with a thick gaseous disk.

TL;DR: In this article, a dynamical classification system for galaxies based on the shapes of their circular velocity curves (CVCs) is presented, where principal component analysis (PCA) is applied to the circular curve shapes to find characteristic features and use a k-means classifier to separate circular curves into classes.

TL;DR: WEAVE as discussed by the authors is a massively multiplexed spectroscopic survey facility for the William Herschel Telescope that will see first light in late 2022, and consists of a 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable integral field units (IFUs), and a single large IFU.

TL;DR: In this article , the authors identify and characterize the sample of ELGs from miniJPAS with a redshift lower than 0 . 35, which is the limit to which the H α emission line can be observed with the J-PAS filter system.

TL;DR: The ALHAMBRA project as mentioned in this paper is a project to gather data to sample a fraction of the Universe with enough precision to follow the evolution of its content and properties with z, a kind of Cosmic Tomography.